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Observations of Ultracool White Dwarfs

Oppenheimer, B. R. and Saumon, D. and Hodgkin, S. T. and Jameson, R. F. and Hambly, N. C. and Chabrier, G. and Filippenko, A. V. and Coil, A. L. and Brown, M. E. (2001) Observations of Ultracool White Dwarfs. Astrophysical Journal, 550 (1). pp. 448-456. ISSN 0004-637X. https://resolver.caltech.edu/CaltechAUTHORS:20120926-112452907

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Abstract

We present new spectroscopic and photometric measurements of the white dwarfs LHS 3250 and WD 0346+246. Along with F351-50, these white dwarfs are the coolest ones known, all with effective temperatures below 4000 K. Their membership in the Galactic halo population is discussed, and detailed comparisons of all three objects with new atmosphere models are presented. The new models consider the effects of mixed H/He atmospheres and indicate that WD 0346+246 and F351-50 have predominantly helium atmospheres with only traces of hydrogen. LHS 3250 may be a double degenerate whose average radiative temperature is between 2000 and 4000 K, but the new models fail to explain this object.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1086/319718DOIArticle
http://iopscience.iop.org/0004-637X/550/1/448/PublisherArticle
https://arxiv.org/abs/astro-ph/0101258arXivDiscussion Paper
ORCID:
AuthorORCID
Filippenko, A. V.0000-0003-3460-0103
Brown, M. E.0000-0002-8255-0545
Additional Information:© 2001 American Astronomical Society. Received 2000 June 15; accepted 2000 November 17. We thank S. R. Kulkarni and J. S. Bloom for their support of this work, M. Irwin for providing us with his spectral data on F351-50, I. N. Reid for sharing the spectrum of LHS 3250, and J. Liebert for useful discussions and suggestions. We also graciously thank the two referees for a thorough job and for insisting that we check the technique in § 5. Financial assistance for this work was provided by NASA through Hubble Fellowship grant HF-01122.01-99A from the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS5-26555. B. R. O. acknowledges FUTDI. D. S. and A. V. F. are supported by NSF grants AST 97-31438 and AST 99-87438, respectively. S. T. H. acknowledges the support of the Particle Physics and Astronomy Research Council. A. L. C. is grateful for a National Science Foundation Graduate Research Fellowship. Part of this work was done under the auspices of ALLIANCE project 00193 RL between the United Kingdom and France. The William Herschel Telescope is operated on the island of La Palma by the Isaac Newton Group in the Spanish Observatorio del Roque de los Muchachos of the Instituto de Astrofisica de Canarias. The W. M. Keck Observatory is operated as a scientific partnership among the California Institute of Technology, the University of California, and NASA; it was made possible by the generous financial support of the W. M. Keck Foundation.
Funders:
Funding AgencyGrant Number
NASA Hubble FellowshipHF-01122.01-99A
NASANAS5-26555
NSFAST 97-31438
NSFAST 99-87438
Particle Physics and Astronomy Research Council (PPARC)UNSPECIFIED
NSF Graduate Research FellowshipUNSPECIFIED
ALLIANCE Project00193
W. M. Keck FoundationUNSPECIFIED
Subject Keywords:stars: fundamental parameters; stars: individual (LHS 3250, WD 0346+246); white dwarfs
Issue or Number:1
Record Number:CaltechAUTHORS:20120926-112452907
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20120926-112452907
Official Citation:Observations of Ultracool White Dwarfs B. R. Oppenheimer et al. 2001 ApJ 550 448
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:34457
Collection:CaltechAUTHORS
Deposited By: Ruth Sustaita
Deposited On:26 Sep 2012 18:48
Last Modified:03 Oct 2019 04:19

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